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arXiv 2403.04517math.NAcs.NA
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适用于所有马赫数与阿尔芬数下理想磁流体动力学的保结构半隐式IMEX有限体积格式

A structure-preserving semi-implicit IMEX finite volume scheme for ideal magnetohydrodynamics at all Mach and Alfvén numbers

Walter Boscheri, Andrea Thomann

AI总结:

本研究提出一种适用于所有马赫数与阿尔芬数的理想MHD无散度半隐式IMEX有限体积格式,通过算子分裂解耦隐式显式项,空间离散保磁场无散性,在多类流动场景下兼具稳定性与效率。

摘要:

我们提出了一种无散度的半隐式有限体积格式,用于模拟理想磁流体动力学(MHD)方程,该格式在所有马赫数与阿尔芬数下,对于由局部输运速度控制的大时间步长均保持稳定。通过算子分裂技术,我们对对流项进行显式处理,同时对流体动压力与磁场贡献项进行隐式积分,由此得到两个解耦的线性隐式系统。隐式部分的线性性通过半隐式时间线性化方法实现。这种结构具有优势,因为借助半隐式隐式-显式龙格-库塔(IMEX-RK)方法族,可以实现时间方向的二阶精度。在空间维度上,我们设计了隐式的单元中心有限差分算子,能够在三维笛卡尔网格上离散地保持磁场的无散度特性。由于隐式项未添加显式数值耗散,且时间步长与尺度无关,该新格式也特别适用于低马赫数流动以及MHD方程的不可压缩极限情况。同样地,高磁化流动可受益于对磁通量的隐式处理,从而提升该新方法的计算效率。对流项采用激波捕捉的二阶有限体积离散方法,以确保所提方法即使在高马赫数流动下也能有效发挥作用。我们针对理想MHD方程的一系列测试用例对新格式进行了基准测试,这些用例覆盖了不同的声学马赫数与阿尔芬马赫数区间,借此评估了新格式的性能与稳定性。

英文摘要:

We present a divergence-free semi-implicit finite volume scheme for the simulation of the ideal magnetohydrodynamics (MHD) equations which is stable for large time steps controlled by the local transport speed at all Mach and Alfvén numbers. An operator splitting technique allows to treat the convective terms explicitly while the hydrodynamic pressure and the magnetic field contributions are integrated implicitly, yielding two decoupled linear implicit systems. The linearity of the implicit part is achieved by means of a semi-implicit time linearization. This structure is favorable as second-order accuracy in time can be achieved relying on the class of semi-implicit IMplicit-EXplicit Runge-Kutta (IMEX-RK) methods. In space, implicit cell-centered finite difference operators are designed to discretely preserve the divergence-free property of the magnetic field on three-dimensional Cartesian meshes. The new scheme is also particularly well suited for low Mach number flows and for the incompressible limit of the MHD equations, since no explicit numerical dissipation is added to the implicit contribution and the time step is scale independent. Likewise, highly magnetized flows can benefit from the implicit treatment of the magnetic fluxes, hence improving the computational efficiency of the novel method. The convective terms undergo a shock-capturing second order finite volume discretization to guarantee the effectiveness of the proposed method even for high Mach number flows. The new scheme is benchmarked against a series of test cases for the ideal MHD equations addressing different acoustic and Alfvén Mach number regimes where the performance and the stability of the new scheme is assessed.

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